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  2. XAUUSD - Wikipedia

    en.wikipedia.org/?title=XAUUSD&redirect=no

    Permanent link; Page information; Cite this page; Get shortened URL; Download QR code; Print/export Download as PDF; Printable version; ... XAUUSD. Add languages ...

  3. W Ursae Majoris - Wikipedia

    en.wikipedia.org/wiki/W_Ursae_Majoris

    It has since become the prototype and eponym for a class of variable stars called W Ursae Majoris variables. [10] This system consists of a pair of stars in a tight, circular orbit with a period of 0.3336 days, or eight hours and 26 seconds. [5] During every orbital cycle, each star eclipses the other, resulting in a decrease in magnitude. The ...

  4. Opposition (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Opposition_(astronomy)

    Seen from a superior planet, an inferior planet on the opposite side of the Sun is in superior conjunction with the Sun. An inferior conjunction occurs when the two planets align on the same side of the Sun. At inferior conjunction, the superior planet is "in opposition" to the Sun as seen from the inferior planet (see the diagram).

  5. A very rare pair of stars is behaving extremely ‘weirdly ...

    www.aol.com/news/very-rare-pair-stars-behaving...

    Pair of stars is a ‘one-in-ten-billion system’, scientists say. Skip to main content. Sign in. Mail. 24/7 Help. For premium support please call: 800-290-4726 more ways to reach us ...

  6. Visual binary - Wikipedia

    en.wikipedia.org/wiki/Visual_binary

    These stars are estimated, via Kepler's third law, to have periods ranging from a few years to thousands of years. A visual binary consists of two stars, usually of a different brightness. Because of this, the brighter star is called the primary and the fainter one is called the companion.

  7. Astronomers spot mysterious object - AOL

    www.aol.com/astronomers-spot-mysterious-object...

    A mysterious object unlike anything ever seen before has been spotted by astronomers. Observations of the “spooky” item showed it releasing a giant burst of energy three times an hour.

  8. NGC 4622 - Wikipedia

    en.wikipedia.org/wiki/NGC_4622

    Analysis of a color-age star formation angle sequence of the Fourier components establishes that the strong outer pair is the leading pair A Fourier component image of the arm pairs is shown with one of the pair of arms marked for the newly discovered inner CCW pair (black dots) as well as one of the already known (CW) outer pair (white dots).

  9. Binary system - Wikipedia

    en.wikipedia.org/wiki/Binary_system

    The most common kinds of binary system are binary stars and binary asteroids, but brown dwarfs, planets, neutron stars, black holes and galaxies can also form binaries. A multiple system is similar but consists of three or more objects, for example triple stars and triple asteroids (a more common term than 'trinary').